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Physics
Astrophysics and Cosmology
Stellar Astronomy and Astrophysics
1. Introduction to Stellar Astrophysics
2. Measurable Properties of Stars
3. Stellar Structure and Atmospheres
4. Star Formation
5. Stellar Evolution: Main Sequence Phase
6. Post-Main-Sequence Evolution
7. Stellar Death and Remnants
8. Explosive Stellar Events
9. Variable Stars
10. Binary and Multiple Star Systems
11. Stellar Nucleosynthesis and Chemical Evolution
Stellar Structure and Atmospheres
Fundamental Physics of Stellar Interiors
Hydrostatic Equilibrium
Pressure Balance
Gravitational Force
Pressure Gradient
Thermal Equilibrium
Energy Generation
Energy Transport
Energy Loss
Mass Conservation
Continuity Equation
Density Distribution
Equation of State
Ideal Gas Law
Radiation Pressure
Degeneracy Pressure
Relativistic Effects
Stellar Structure Equations
Mass Conservation Equation
Hydrostatic Equilibrium Equation
Energy Generation Equation
Energy Transport Equation
Boundary Conditions
Central Conditions
Surface Conditions
Energy Generation Mechanisms
Nuclear Fusion Processes
Proton-Proton Chain
CNO Cycle
Triple-Alpha Process
Advanced Burning Stages
Energy Generation Rates
Temperature Dependence
Composition Dependence
Neutrino Production
Neutrino Types
Energy Loss Mechanisms
Energy Transport Mechanisms
Radiative Transport
Radiative Diffusion Equation
Opacity Sources
Bound-Bound Transitions
Bound-Free Transitions
Free-Free Transitions
Electron Scattering
Mean Opacity
Rosseland Mean Opacity
Convective Transport
Convective Instability
Schwarzschild Criterion
Ledoux Criterion
Mixing Length Theory
Convective Zones
Conductive Transport
Electron Conduction
Importance in Dense Objects
Stellar Models and Structure
Polytropic Models
Polytropic Equation of State
Lane-Emden Equation
Polytropic Index
Standard Solar Model
Solar Structure
Central Conditions
Composition Profile
Stellar Evolution Models
Numerical Integration
Evolutionary Tracks
Stellar Lifetimes
Helioseismology
Solar Oscillations
p-modes and g-modes
Internal Structure Probes
Stellar Atmospheres
Atmospheric Structure
Temperature-Pressure Profile
Photosphere Definition
Chromosphere and Corona
Radiative Transfer
Radiative Transfer Equation
Source Function
Optical Depth
Formal Solution
Line Formation
Excitation and Ionization
Saha Equation
Boltzmann Equation
Line Strength
Model Atmospheres
Plane-Parallel Models
Local Thermodynamic Equilibrium
Non-LTE Models
Three-Dimensional Models
Stellar Winds and Mass Loss
Wind Driving Mechanisms
Radiation Pressure
Thermal Pressure
Magnetic Fields
Mass Loss Rates
Terminal Velocities
Observational Signatures
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2. Measurable Properties of Stars
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4. Star Formation